Microcontinent formation around Australia
Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen...
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ftqueensland:oai:eprints.qut.edu.au:234263 2024-02-04T09:55:42+01:00 Microcontinent formation around Australia Gaina, C. Müller, R. D. Brown, B. Ishihara, T. Hillis, R. R. Muller, R. D. 2003 https://eprints.qut.edu.au/234263/ unknown Geological Society of America doi:10.1130/0-8137-2372-8.405 Gaina, C., Müller, R. D., Brown, B., & Ishihara, T. (2003) Microcontinent formation around Australia. In Hillis, R. R. & Muller, R. D. (Eds.) Evolution and Dynamics of the Australian Plate. Geological Society of America, United States of America, pp. 405-416. https://eprints.qut.edu.au/234263/ 2003 Geological Society of America, Inc. This work is covered by copyright. Unless the document is being made available under a Creative Commons Licence, you must assume that re-use is limited to personal use and that permission from the copyright owner must be obtained for all other uses. If the document is available under a Creative Commons License (or other specified license) then refer to the Licence for details of permitted re-use. It is a condition of access that users recognise and abide by the legal requirements associated with these rights. If you believe that this work infringes copyright please provide details by email to qut.copyright@qut.edu.au Evolution and Dynamics of the Australian Plate Hot spots Microcontinent Riffing Sea-floor spreading Chapter in Book, Report or Conference volume 2003 ftqueensland https://doi.org/10.1130/0-8137-2372-8.405 2024-01-09T00:09:21Z Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen Plateau), and possibly fragments of the Lord Howe Rise and Norfolk Ridge, and the Wallaby Plateau. We review their history of formation, and propose that the mechanisms that led to their isolation were mostly plume-related. Tasman Sea continental fragments formed by ridge jumps onto adjacent continental margins after sea-floor spreading in the southern Tasman Sea commenced. The East Tasman Plateau was separated from the Lord Howe Rise at about chron 34 (83 Ma) and the Gilbert Seamount Complex rifted off the South Tasman Rise at roughly 77 Ma, by ridge jumps in opposing directions. Evidence for thermal anomalies under the central Lord Howe Rise, Ross Sea and possible eastern Australian margin explain ridge jumps that led to the isolation of the East Tasman Plateau, Gilbert Seamount and possibly the northern Lord Howe Rise and Dampier Ridge. In the central Indian Ocean, spectacular exposures of granite make the Seychelles a type example of a microcontinent. As in the Tasman Sea, ridge-plume interactions have been responsible for separating a thinned continental sliver from a large continent (India). Elan Bank, as part of the Kerguelen Plateau, represents another example of a continental fragment in the Indian Ocean. Newly identified M-sequence anomalies in the Enderby Basin, off Antarctica, suggest that this microcontinent was detached from India no earlier than 124 Ma when a northward ridge jump towards the Kerguelen plume may have isolated Elan Bank. This Interpretation implies that a mantle thermal anomaly due to the incipient Kerguelen plume pre-dated the Rajmahal Traps, emplaced at about 118 Ma, by ∼6 million years. An early Kerguelen hot-spot position north of Elan Bank, with subsequent southward migration, is also ... Book Part Antarc* Antarctica Ross Sea Queensland University of Technology: QUT ePrints Ross Sea Kerguelen Indian South Tasman Rise ENVELOPE(148.000,148.000,-47.500,-47.500) Elan Bank ENVELOPE(67.000,67.000,-56.750,-56.750) Gilbert Seamount ENVELOPE(-150.083,-150.083,52.833,52.833) |
institution |
Open Polar |
collection |
Queensland University of Technology: QUT ePrints |
op_collection_id |
ftqueensland |
language |
unknown |
topic |
Hot spots Microcontinent Riffing Sea-floor spreading |
spellingShingle |
Hot spots Microcontinent Riffing Sea-floor spreading Gaina, C. Müller, R. D. Brown, B. Ishihara, T. Microcontinent formation around Australia |
topic_facet |
Hot spots Microcontinent Riffing Sea-floor spreading |
description |
Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen Plateau), and possibly fragments of the Lord Howe Rise and Norfolk Ridge, and the Wallaby Plateau. We review their history of formation, and propose that the mechanisms that led to their isolation were mostly plume-related. Tasman Sea continental fragments formed by ridge jumps onto adjacent continental margins after sea-floor spreading in the southern Tasman Sea commenced. The East Tasman Plateau was separated from the Lord Howe Rise at about chron 34 (83 Ma) and the Gilbert Seamount Complex rifted off the South Tasman Rise at roughly 77 Ma, by ridge jumps in opposing directions. Evidence for thermal anomalies under the central Lord Howe Rise, Ross Sea and possible eastern Australian margin explain ridge jumps that led to the isolation of the East Tasman Plateau, Gilbert Seamount and possibly the northern Lord Howe Rise and Dampier Ridge. In the central Indian Ocean, spectacular exposures of granite make the Seychelles a type example of a microcontinent. As in the Tasman Sea, ridge-plume interactions have been responsible for separating a thinned continental sliver from a large continent (India). Elan Bank, as part of the Kerguelen Plateau, represents another example of a continental fragment in the Indian Ocean. Newly identified M-sequence anomalies in the Enderby Basin, off Antarctica, suggest that this microcontinent was detached from India no earlier than 124 Ma when a northward ridge jump towards the Kerguelen plume may have isolated Elan Bank. This Interpretation implies that a mantle thermal anomaly due to the incipient Kerguelen plume pre-dated the Rajmahal Traps, emplaced at about 118 Ma, by ∼6 million years. An early Kerguelen hot-spot position north of Elan Bank, with subsequent southward migration, is also ... |
author2 |
Hillis, R. R. Muller, R. D. |
format |
Book Part |
author |
Gaina, C. Müller, R. D. Brown, B. Ishihara, T. |
author_facet |
Gaina, C. Müller, R. D. Brown, B. Ishihara, T. |
author_sort |
Gaina, C. |
title |
Microcontinent formation around Australia |
title_short |
Microcontinent formation around Australia |
title_full |
Microcontinent formation around Australia |
title_fullStr |
Microcontinent formation around Australia |
title_full_unstemmed |
Microcontinent formation around Australia |
title_sort |
microcontinent formation around australia |
publisher |
Geological Society of America |
publishDate |
2003 |
url |
https://eprints.qut.edu.au/234263/ |
long_lat |
ENVELOPE(148.000,148.000,-47.500,-47.500) ENVELOPE(67.000,67.000,-56.750,-56.750) ENVELOPE(-150.083,-150.083,52.833,52.833) |
geographic |
Ross Sea Kerguelen Indian South Tasman Rise Elan Bank Gilbert Seamount |
geographic_facet |
Ross Sea Kerguelen Indian South Tasman Rise Elan Bank Gilbert Seamount |
genre |
Antarc* Antarctica Ross Sea |
genre_facet |
Antarc* Antarctica Ross Sea |
op_source |
Evolution and Dynamics of the Australian Plate |
op_relation |
doi:10.1130/0-8137-2372-8.405 Gaina, C., Müller, R. D., Brown, B., & Ishihara, T. (2003) Microcontinent formation around Australia. In Hillis, R. R. & Muller, R. D. (Eds.) Evolution and Dynamics of the Australian Plate. Geological Society of America, United States of America, pp. 405-416. https://eprints.qut.edu.au/234263/ |
op_rights |
2003 Geological Society of America, Inc. This work is covered by copyright. Unless the document is being made available under a Creative Commons Licence, you must assume that re-use is limited to personal use and that permission from the copyright owner must be obtained for all other uses. If the document is available under a Creative Commons License (or other specified license) then refer to the Licence for details of permitted re-use. It is a condition of access that users recognise and abide by the legal requirements associated with these rights. If you believe that this work infringes copyright please provide details by email to qut.copyright@qut.edu.au |
op_doi |
https://doi.org/10.1130/0-8137-2372-8.405 |
_version_ |
1789959807270125568 |